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arXiv 1405.2187astro-ph.COhep-ph
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随机$δN$形式中曲率扰动的非微扰方法

Non-perturbative approach for curvature perturbations in stochastic-$δN$ formalism

Tomohiro Fujita, Masahiro Kawasaki, Yuichiro Tada

摘要:

在我们的前一篇文章中,我们提出了一种新的算法,用随机方法计算暴胀宇宙中曲率扰动的功率谱。由于该算法不需要对暴胀子场进行超视界尺度的微扰展开,因此即使在高度随机的情况下也有效。例如,当曲率扰动非常大或曲率扰动的非高斯性相当大时,扰动展开可能会崩溃,但我们的算法能够计算曲率扰动。本文将其应用于两个著名的通货膨胀模型,混沌和混合通货膨胀。特别是对于混合暴胀,虽然势在临界点附近非常平坦,标准的微扰计算是有问题的,我们成功地计算了曲率微扰。

英文摘要:

In our previous paper, we have proposed a new algorithm to calculate the power spectrum of the curvature perturbations generated in inflationary universe with use of the stochastic approach. Since this algorithm does not need the perturbative expansion with respect to the inflaton fields on super-horizon scale, it works even in highly stochastic cases. For example, when the curvature perturbations are very large or the non-Gaussianities of the curvature perturbations are sizable, the perturbative expansion may break down but our algorithm enables to calculate the curvature perturbations. We apply it to two well-known inflation models, chaotic and hybrid inflation, in this paper. Especially for hybrid inflation, while the potential is very flat around the critical point and the standard perturbative computation is problematic, we successfully calculate the curvature perturbations.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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